K. Sigsbee1, C. Cattell1, R. Lysak1,
F. Mozer2, C. Carlson2, R. Ergun2,
J. McFadden2, K. Tsuruda3, T. Yamamoto3,
T. Okada4, S. Kokubun5, D. Fairfield6,
R. Strangeway7, G. Parks8, M. Brittnacher8
1School of Physics and Astronomy, University of Minnesota,
Minneapolis, MN USA
2University of California, Berkeley
3ISAS
4Toyama Prefectural University
5STELAB, Nagoya University
6NASA/GSFC
7UCLA
8University of Washington, Seattle, WA
Abstract. During January and February 1997, a
number of conjunctions between the FAST and
Geotail satellites occurred when FAST was at apogee
above the nightside auroral zone in the northern
hemisphere and Geotail was close to midnight near the
equatorial plane. These events provided an
opportunity to examine physical processes connecting
the magnetotail at 20 to 40 RE to the auroral zone
during substorms and quiet times. We present results
from conjunctions on January 18, 1997 [Sigsbee et al.,
1998] and February 3, 1997. Images from Polar were
available during both events. Comparison of waves
observed by Geotail and FAST on January 18
provided evidence for magnetosphere-ionosphere
coupling via Alfvén waves, as well as the near
simultaneous occurrence of waves in other frequency
bands. Similar results were obtained during the
February 3, 1997 conjunction. These observations are
significant to the verification and further development
of magnetosphere-ionosphere coupling models.